Theia 2541

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0.38 UTI
0.3
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2541 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 202.192 -64.252 0.494 -4.658 -2.634 4.657
Hunt & Reffert 2024 202.193 -64.266 0.496 -4.695 -2.633 –
Cavallo et al. 2024 202.224 -64.274 0.496 – – –
Hunt & Reffert 2023 202.193 -64.266 0.496 -4.695 -2.633 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 155* – –
Cavallo et al. 2024 1.78 0.95 – 35 -0.170 – – –
Hunt & Reffert 2023 1.87 0.60 0.41 62 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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